VOLCANIC ERUPTIONS AT PLATE BOUNDARIES - Career Paths for African-American Students - Eos.org
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VOL. 97 • NO. 13 • 1 JUL 2016 Career Paths for African-American Students Did Solar Flares Cook Up Life? High Energy Growth Forecast Through 2040 VOLCANIC ERUPTIONS AT PLATE BOUNDARIES
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Earth & Space Science News Contents 1 JULY 2016 PROJECT UPDATE VOLUME 97, ISSUE 13 9 Creating Career Paths for African-American Students in Geosciences A new initiative at Stony Brook University teaches marketable skills, engages students in research projects, and fosters professional career tracks of underrepresented minorities. NEWS 6 Advisory Panel Calls for Large Increase for Ocean Exploration The recently established Ocean Exploration Advisory Board also urged the National Oceanic and Atmospheric Administration 12 to increase its role in federal coordination of exploration. COVER RESEARCH SPOTLIGHT Understanding Volcanic Eruptions Where Plates Meet 31 Researchers Attribute Human Influence on Climate Back to 1930s A new project clarifies the relationships between tectonics and A new study finds that humans likely have volcanic systems and how they influence hazards on Italy’s Mount triggered the past 16 record-breaking hot Etna and Vulcano and Lipari islands. years on Earth, up to 2014. Earth & Space Science News Eos.org // 1
Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ brichman@agu.org Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl.caltech.edu .com Chicago, Chicago, Ill., USA; cstein@uic.edu José D. Fuentes David Halpern Department of Meteorology, Jet Propulsion Laboratory, Pennsylvania State Pasadena, Calif., USA; University, University davidhalpern29@gmail Park, Pa., USA; .com juf15@meteo.psu.edu Editorial Advisory Board M. Lee Allison, Earth and Space John W. Lane, Near-Surface Geophysics Science Informatics Jian Lin, Tectonophysics Mark G. Flanner, Atmospheric Figen Mekik, Paleoceanography Sciences and Paleoclimatology Nicola J. Fox, Space Physics Jerry L. Miller, Ocean Sciences and Aeronomy Michael A. Mischna, Planetary Sciences Steve Frolking, Biogeosciences Thomas H. Painter, Cryosphere Sciences Edward J. Garnero, Study of the Philip J. Rasch, Global Environmental 30 Earth’s Deep Interior Michael N. Gooseff, Hydrology Change Eric M. Riggs, Education Brian C. Gunter, Geodesy Adrian Tuck, Nonlinear Geophysics Kristine C. Harper, History Sergio Vinciguerra, Mineral 18–28 AGU News of Geophysics and Rock Physics Susan E. Hough, Natural Hazards Andrew C. Wilcox, Earth and Planetary How on Earth to Decide Where on Emily R. Johnson, Volcanology, Surface Processes Mars to Land?; Recognizing 2015 Geochemistry, and Petrology Earle Williams, Atmospheric Keith D. Koper, Seismology and Space Electricity Reviewers for AGU. Robert E. Kopp, Geomagnetism Mary Lou Zoback, Societal Impacts and Paleomagnetism and Policy Sciences 30–32 Research Spotlight Staff Streamlining Rapid Tsunami Production and Design: Faith A. Ishii, Production Manager; Melissa A. Tribur, Senior Production Specialist; Liz Castenson, Editorial and Production Coordinator; Elizabeth Forecasting; Researchers Attribute Jacobsen, Production Intern; Yael Fitzpatrick, Manager, Design and Branding; Valerie Human Influence on Climate Bassett and Travis Frazier, Electronic Graphics Specialists Back to 1930s; The Role of Water Editorial: Peter L. Weiss, Manager/Senior News Editor; Mohi Kumar, Scientific Content Editor; Randy Showstack, Senior News Writer; JoAnna Wendel, News Writer; in Earth’s Tectonic Plumbing Amy Coombs and Elizabeth Deatrick, Editorial Interns Systems; Martian Carbonates Marketing: Angelo Bouselli, Marketing Program Manager; Jamie R. Liu, Manager, 7 Spotted by the Orbiter; Improving Marketing Advertising: Christy Hanson, Manager; Tel: +1-202-777-7536; Email: advertising@ the Identification of Extreme U.S. agu.org Precipitation Trends. 3–6 News ©2016. American Geophysical Union. All Rights Reserved. Material in this issue may be photocopied by individual scientists for research or classroom use. Permission is also High Energy Growth, Fossil Fuel 33–35 Positions Available granted to use short quotes, figures, and tables for publication in scientific books and Dependence Forecast Through Current job openings in the Earth journals. For permission for any other uses, contact the AGU Publications Office. 2040; Did Solar Flares Cook Up Life and space sciences. Eos (ISSN 0096-3941) is published semi-monthly, on the 1st and 15th of the month by the American Geophysical Union, 2000 Florida Ave., NW, Washington, DC 20009, on Earth?; Storms Cause Infrequent USA. Periodical Class postage paid at Washington, D. C., and at additional mailing offices. POSTMASTER: Send address changes to Member Service Center, 2000 Turbulence for Aircraft, New Study 36 Postcards from the Field Florida Ave., NW, Washington, DC 20009, USA. Finds; Advisory Panel Calls for A view of Edinburg of the Seven Member Service Center: 8:00 a.m.–6:00 p.m. Eastern time; Tel: +1-202-462-6900; Large Increase for Ocean Seas, the main settlement on Fax: +1-202-328-0566; Tel. orders in U.S.: 1-800-966-2481; Email: service@agu.org. Exploration. Tristan da Cunha, an island in the Use AGU’s Geophysical Electronic Manuscript Submissions system southern Atlantic Ocean. to submit a manuscript: http://eos-submit.agu.org. 7–8 Meeting Reports Views expressed in this publication do not necessarily reflect official positions of the American Geophysical Union unless expressly stated. Extending Recent Seismic Imaging On the Cover Christine W. McEntee, Executive Director/CEO Successes to South America; Lava flows from Italy’s Mount Etna Norway and Cuba Evaluate Bilateral on the island of Sicily.Credit: Getty Climate Research Results. Images/DEA/F. Barbagallo facebook.com/AmericanGeophysicalUnion @AGU_Eos linkedin.com/company/american-geophysical-union youtube.com/user/AGUvideos 2 // Eos 1 July 2016
NEWS High Energy Growth, Fossil Fuel Dependence Forecast Through 2040 T he world’s energy consumption will The EIA report includes some details from through 2040 coming from China, India, Indo- increase by 48% between 2012 and 2040, the Paris agreement but notes uncertainty nesia, and other developing countries in Asia. with fossil fuels accounting for more about whether countries will meet their cli- EIA’s Sieminski said at the briefing that than 75% of world energy use in 2040, accord- mate targets. EIA head Adam Sieminski said at some global issues increase the uncertainty of ing to the U.S. Energy Information Adminis- the briefing that incorporating country cli- the forecast, including economic growth rates tration (EIA). Fossil fuels supplied 83% of mate pledges into the forecast “is compli- in China and elsewhere, technological innova- global energy demand in 2015. cated” but that the next IEO in 2017 “will tions, the future of nuclear generating capac- Energy-related carbon dioxide (CO2) emis- probably have more to say” about those com- ity, the implementation and strength of cli- sions will increase 34% during that time span, mitments. mate policies, and unrest in oil-producing with annual emissions rising from 32 billion countries. metric tons in 2012 to 43 billion metric tons in Renewables on a Fast Track 2040, the agency projects. Coal will continue According to the EIA, renewable energy will be to generate the most energy-related CO2 the fastest growing energy source, climbing by By Randy Showstack, Staff Writer emissions worldwide, although its share will 2.6% per year, and decline from 43% in 2012 to 38% in 2040, nuclear energy will according to International Energy Outlook 2016 increase from 4% to (IEO), an EIA report released in May at a brief- 6% of the energy pie. ing in Washington, D. C. (see http://bit.ly/ Coal, which the EIAreport-2016). report deemed “the U.S. Energy Information Administration world’s slowest Meeting Climate Targets growing energy The numbers in the 11 May report “indicated source,” will rise by the challenge for the world to reduce global about 0.6% per year. CO2 emissions substantially by 2040 and In 2040, coal, natural beyond,” Jan Mares, senior policy adviser gas, and renewables with Resources for the Future, told Eos. The each will contribute organization is a Washington, D. C.–based just under 30% of the think tank that focuses on natural resources world’s net electricity Fossil fuels continue to play a key role in meeting energy demands through 2040, and environment issues. Other energy and generation, the according to EIA’s energy outlook. Btu = British thermal unit (~1055 joules). climate analysts said the new projections report states. indicate that the means of energy production Cleetus told Eos need to shift soon if the world is to achieve that the EIA forecast climate targets. likely underestimates “The low hanging fruit, which is substitut- contributions from ing [natural] gas for coal, seems to be on track renewables and and looks pretty robust,” David Goldwyn, energy efficiency and president of Goldwyn Global Strategies, an does not address the international energy advisory consultancy, implications of rising told Eos. “But it’s also clear that we need a big methane emissions technological step change to get to 2 degrees associated with natu- [Celsius] or even frankly to stabilize emissions ral gas use. The fore- at the level we have right now. We’re not there cast “illustrates the U.S. Energy Information Administration yet, and the growth in renewables, which is pitfalls of an over mostly hydro, is not going to get us there.” reliance on natural “A business-as-usual scenario, with no new gas as we shift away policies beyond those that exist right now, from coal,” she also would be disastrous from a climate perspec- said. tive,” Rachel Cleetus, lead economist and cli- mate policy manager for the Union of Con- Asian Energy cerned Scientists, told Eos. “The good news is Consumption we are not in a business-as-usual world,” she Continues Rapid said, citing the recent Paris climate agreement Growth The energy outlook forecasts that energy-related carbon dioxide emissions will increase (see http://bit.ly/COP21-signed) and commit- The outlook forecasts 34% between 2012 and 2040. This chart shows historical and projected world energy- ments by major emitters to cut carbon and more than half of the related carbon dioxide emissions by fuel type, from 1990 through 2040, in billions of increase renewables and efficiency. energy growth metric tons. Earth & Space Science News Eos.org // 3
NEWS Did Solar Flares Cook Up an atmospheric model using scientists’ best estimates of concentrations of different gases Life on Earth? in the atmosphere 4 billion years ago; at that time, molecular nitrogen (N2) was a main component of the atmosphere, along with carbon dioxide (CO2), methane, and water vapor. They then subjected their model atmo- S pace weather today threatens our satel- they released huge bursts of radiation and sphere to simulated super solar flares that lites, our space station, and our tele- magnetic energy, Airapetian said. These they suspect the young Sun produced—some- communications, but 4 billion years bursts, called super flares, can be quite fre- times multiple times per day—and studied ago, large solar flares and their associated quent—observers see some of these stars what happened to the model atmosphere. energetic particles could have provided the belching out 10 of these super flares in a day. The researchers found that energetic parti- planet its first ingredients for life. Using these observations, Airapetian and cles associated with super solar flares com- Researchers at NASA have found that when his team extrapolated that when our Sun was pressed Earth’s magnetic field and created the Sun was about half a billion huge gaps at the poles, which years old, large solar flares— allowed highly energetic solar larger than any recorded by protons to pierce the atmosphere. humans—could have changed the Those protons knocked electrons very chemistry of Earth’s atmo- around like bowling pins, which sphere. What’s more, bombard- knocked into more electrons in an ment of the planet by high- “avalanche of electrons,” Airape- energy particles from those jets of tian said. This “avalanche” ion- superhot solar plasma might have ized atoms and tore apart existing prompted organic molecules con- carbon dioxide, methane, and sidered precursors to life to form water vapor molecules, as well as from simpler inorganic molecules molecular nitrogen—an then abundant on primordial extremely unreactive and strongly Earth. bonded molecule, Airapetian said. One of the types of molecules The resulting highly reactive sub- that could have newly formed stances acted as building blocks back then is a potent greenhouse for new substances. gas. Thus the findings may illu- “Once you have those building minate a long-standing mystery blocks, you have a fertile environ- about how Earth could have been ment to start reactive chemistry,” so warm and hospitable to life at a Airapetian said. time when, despite the solar One molecule that may have NASA/Goddard/SDO flares, the Sun was significantly formed in Earth’s infant atmo- less bright than it is today. sphere was hydrogen cyanide “To make organic stuff out of (HCN)—a molecule considered inorganic stuff, you need a lot of vital to life’s origins (see http:// energy,” said Vladimir Airapetian, bit.ly/origins-solution). The an astrophysicist at NASA’s God- Solar flares, the largest explosions in our solar system, took place much more frequently newly formed HCN in a turbulent dard Space Flight Center in 4 billion years ago than today, bombarding Earth with energetic protons and radiation. atmosphere would have dissolved Greenbelt, Md. Airapetian, the into clouds and rained out, Aira- lead author on a paper about the petian said, likely interacting with research published recently in Nature Geosci- about half a billion years old, it likely bom- water to form other molecules necessary for ence, explained that perhaps that energy came barded Earth with a constant stream of super life, like formaldehyde, amino acids, and com- from solar flares (see http://bit.ly/super-flares solar flares—up to 5 times larger than the plex sugars. -life). infamous Carrington event in 1859 (see http:// This barrage of solar flares could have been The new findings may also affect how bit.ly/Carrington-Superstorm). That magnetic like a worldwide version of the Miller-Urey researchers assess the prospects for life on storm, the largest ever recorded by humans, experiments, Airapetian said, when scientists worlds orbiting other stars by putting a new knocked out telegraph operations around the sparked artificial “atmospheres,” full of gases emphasis on young, active stars. world and sent the aurora borealis streaming like carbon dioxide, methane, ammonia, and as far south as Miami, Fla. A similar event water vapor, with electrical charges and found Solar Flares from Young Suns today would cause trillions of dollars in dam- that this gave rise to amino acids, one of the For almost 10 years, NASA’s Kepler telescope age to telecommunications, Airapetian said, building blocks of life (see http://bit.ly/M has been closely observing stars across the and throw cities around the world into cata- -Uexperiment-video). galaxy and the exoplanets that orbit them. strophic power outages. Previous observations by the telescope have Faint Young Sun revealed that stars similar to our Sun and All About Energy Another molecule that may have formed in younger than a billion years old temporarily To find out how these super flares may have this energized atmosphere was nitrous oxide brightened from time to time, indicating that affected infant Earth, the researchers created (N2O). You’ve probably heard this gas called 4 // Eos 1 July 2016
NEWS laughing gas for its ability to calm even the most anxious dental patients. Storms Cause Infrequent Turbulence However, “laughing gas is not a laughing matter for early Earth,” Airapetian said. This for Aircraft, New Study Finds nitrous oxide was important for young Earth, he said. Although the Sun persistently showered Earth in solar flares 4 billion years ago, it was 30% dimmer than it is now. Earth should have been a ball of ice, Airapetian said, but evidence shows there was liquid water (life cannot form without it). So how did Earth heat up enough to sustain this water? Scientists call this the iStock.com/RayOneMedia faint young Sun paradox (see http://bit.ly/ Reviews-Geophys-FaintSun). Today carbon dioxide drives warming of Earth’s atmosphere in a big way, but 4 billion years ago, if there had been enough CO2 in the atmosphere to heat the planet, Earth’s oceans would have been too acidic for life to evolve, Turbulence affecting air travel results from storms only about a sixth as often as other studies have estimated, new Airapetian said. Nitrous oxide, however, data suggest. warms the atmosphere 300 times more effec- tively than CO2. Even though N2O was—and P remains today—a small portion of the atmo- ast studies have found that convective sensors can triangulate the location of light- sphere, perhaps it played the major role in storms, like thunderstorms, cause a ning strikes. The areas with the most light- heating the planet, Airapetian and his col- large portion of turbulence that plagues ning strikes represented the centers of con- leagues propose in their 23 May paper. commercial airliners. Using those findings, a vective storms, the researchers said. The new study “is a viable additional piece research team in the United Kingdom recently Comparing these data with more commonly in the long-scattered puzzle of how adequate set out to create an automated system for tur- used indicators of turbulence sources, includ- supplies of biologically available nitrogen and bulence detection that relies on lightning sen- ing satellite imagery of clouds and velocity a warm atmosphere were maintained during sors to alert airlines of dangerous winds. data from aboard airplanes, allowed the Earth’s earliest history,” said Timothy Lyons, Now, following the first tests of this new researchers to study the effects of turbulence a biogeochemist at the University of Califor- system, the researchers from the Met Office in from those storms on airplanes flying near nia, Riverside, who was not involved in the Exeter have found that airplanes flying near them. research. “This is an exciting idea that could convective storms experience much less tur- Sharman said he holds some doubts about kill two birds with one stone.” bulence than they expected: Just 14% of turbu- the accuracy of lightning as a storm detection lence events were associated with convective method, saying that lightning may not always Implications for Extraterrestrial Life storms. be concentrated in the center of a storm. Beyond offering new insight into how early This finding sharply contrasts with results Moreover, he said, it’s not clear “just because Earth might have become a crucible for life, of some previous studies that estimated that there’s lightning that there’s turbulence.” the new work has broader implications, Aira- between 82% and 86% of turbulence encoun- The new study’s disagreement with pre- petian said. “Our model expands the tradi- ters were associated with convective storms. vailing wisdom “may also indicate that con- tional definition of habitable zones of habit- The authors of the new study (see http://bit.ly/ vection is relatively less important as a source able exoplanets,” he noted. Now scientists can JAMC-turbulence) suggest that other sources of turbulence over Europe and the northeast- also consider exoplanets that may be orbiting of turbulence, such as winds forced up over ern Atlantic than over other regions (such as young, energetic, Sun-like stars, where suffi- mountain ranges, should receive a greater North America and the tropics),” the team cient energy could become available to make share of researchers’ attention in the future. noted in the paper’s conclusions. Many prior organic molecules out of inorganic molecules. The Met Office team published its results in turbulence studies took place over North In the habitable zone around a star, liquid the May issue of the Journal of Applied Meteo- America. water can persist on a planet’s surface, but a rology and Climatology. However, Sharman said that it’s unlikely new type of habitable zone could be termed Some turbulence researchers found the that significantly less turbulence occurs over the “biogenic zone,” Airapetian said. There numbers surprising. The frequency of turbu- Europe compared with North America. not only does water stay liquid, “but also the lence from convective storms “seems a little The Met Office team ran its tests for two planetary atmosphere receives enough energy low, at least compared to over the continental 6-month periods (May through October) in to make biomolecules of life, setting a path- U.S.,” said Robert Sharman, an atmospheric 2013 and 2014. The researchers noted that a way to [forming] RNA and DNA.” scientist with the National Center for Atmo- future study “over a significantly longer time He and his colleagues are also currently spheric Research in Boulder, Colo., who was period” would help test the validity of the studying how super solar flares could have not involved with the new study. patterns they found. affected Mars. The Met Office researchers used an uncon- ventional tool to pinpoint turbulent loca- tions: a network of lightning sensors scat- By Elizabeth Deatrick, Writer Intern; email: By JoAnna Wendel, Staff Writer tered across Europe and North Africa. These edeatrick@agu.org Earth & Space Science News Eos.org // 5
NEWS Advisory Panel Calls for Large coordinating ocean exploration among federal agencies. The board’s letter calls upon NOAA Increase for Ocean Exploration also to work more vigorously to draw in federal and private funding for ocean exploration and to provide some specific ocean observations that are needed in certain regions, including the Arctic, among other measures. NOAA, through its Office of Ocean Exploration and Research (OER), coordinates the only federal program to systematically explore the oceans. Board Chair Sets a Higher Funding Goal “America’s future depends on understanding the oceans,” the OEAB mentioned in a state- ment that the group approved at its recent meeting about why more exploration is needed. “We explore the oceans because their NOAA Office of Ocean Exploration and Research health and resilience are vital to our economy and to our lives: climate, food, shipping, national security, medicine, and natural resources,” the summary also said. The U.S. national ocean exploration pro- gram “probably should be at least $200 mil- lion,” Vice Admiral Paul G. Gaffney II, U.S. Navy (Ret.), chair of the OEAB, told Eos in an interview. “I just think it hasn’t earned all the respect that it’s due yet.” The White House requested $19 million for The Okeanos Explorer carries out scientific research of the ocean for the National Oceanic and Atmospheric Administration. FY 2017, the same amount it requested for FY 2016, whereas the FY 2018 budget request, already in early formulation, shows hints of I n the United States, federal funding for lished OEAB, an independent U.S. federal some improvement, according to OEAB (see exploration of the nation’s offshore exclu- advisory committee, in 2014 to provide advice http://bit.ly/OEABchair-slides). sive economic zone and of the global ocean on ocean exploration to NOAA and the nation should be much higher than currently bud- geted, according to a recent letter that the (see http://bit.ly/OEABsite). The ocean exploration program within “Given the budget Ocean Exploration Advisory Board (OEAB) sent NOAA received approximately $32 million for resources that we have, to the National Oceanic and Atmospheric fiscal year (FY) 2016. However, in a 27 April Administration (NOAA). The agency estab- letter to NOAA’s chief scientist and other can we accomplish agency officials, the board wrote that pre- everything?” Call for Ocean Discovery Lecturers vious national stud- ies “envision annual funding of $75 mil- Gaffney said that NOAA, an agency within The U.S. Science Support Program (USSSP) is seeking dynamic speakers to lion to execute ocean the Department of Commerce, doesn’t have convey the excitement of the International Ocean Discovery Program exploration activi- the same budgeting flexibility as the Depart- (IODP) to geoscience communities and the United States public. ties.” A report of the ment of Defense or even NASA and that it Since 1991, more than 750 presentations have been made to audiences at President’s Panel for might be difficult to move funding around. U.S. colleges, universities, and informal learning centers. Your help is Ocean Exploration Alan Leonardi, NOAA’s OER director, called requested to identify scientists interested in participating in the Ocean issued in 2000 rec- the advice to the agency “positive.” He did not Discovery Lecture Series Program during the 2017-2018 academic year. Lectures focus on the discoveries and results of scienti�ic ocean drilling ommended that comment specifically on budget levels but told and are primarily aimed at undergraduate and graduate students, amount (see http:// Eos that “there are a lot of competing museums, science departments, and the scienti�ically literate public. bit.ly/ocean-panel demands for federal resources.” If you or someone you know is interested in becoming an Ocean Discovery -report). Leonardi said he agrees with much of the Lecturer, email their name, institution, and potential lecture topic to the The board’s letter board’s advice to NOAA. “My reservations are USSSP Of�ice (usssp@LDEO.columbia.edu) by the nomination deadline of and a related one that given the budget resources that we have, July 22, 2016. sent to NOAA admin- can we accomplish everything?” he said. He istrator Kathryn Sul- added that NOAA officials will respond to the Deadline: livan the same day also recommend that board after reviewing the letters. July 22, 2016 NOAA play a more proactive role in By Randy Showstack, Staff Writer 6 // Eos 1 July 2016
MEETING REPORT Extending Recent Seismic Imaging vices and potential collaborations available from the IRIS community. Successes to South America The workshop concluded with all partici- pants having a fundamental understanding of the ANT method and the ability to continue Ambient Noise Tomography Workshop (MIMOSA) applying this method at their home institu- Tucson, Arizona, 17–23 January 2016 tions. To extend the ANT method across the South American continent, participants were encouraged to seek out additional collabora- tions with neighboring countries. In view of the recent increase in broadband seismic networks in South America and grow- ing interest among their operators, attendees agreed that more of these kinds of workshops are needed. A unique opportunity exists for researchers to cultivate this growing scientific interest through mutually beneficial interna- tional collaborations, leading to a better understanding of the geodynamic and tectonic Klaus Balzano, CC BY-NC 2.0 (http://bit.ly/ccbync2-0) history of the South American continent. For more on this meeting, see http://bit.ly/ 1sKuDvC. By Kevin M. Ward, Jonathan R. Delph, and Susan L. Beck, Geosciences Department, Uni- versity of Arizona, Tucson; email: wardk@email .arizona.edu Torres del Paine, Chile. What structures underlie these mountains and other features in South America? O ne of the main scientific goals of the As part of the MIMOSA project, research- EarthScope transportable array (see ers from five South American countries http://www.earthscope.org/) is to along with other visiting researchers from investigate the structure, dynamics, and tec- around the world gathered at the University tonic history of the North American continent. of Arizona in January for a weeklong work- But what about South America? shop on ambient noise tomography (ANT). A Although South America does not have the seismic imaging technique refined by scien- seismic station distribution and near-real- tists working on EarthScope, ANT methods time data access associated with a transport- allow scientists to use low-amplitude back- able array, a developing collection of national ground seismic noise to create images of the broadband seismic networks is beginning to crust and uppermost mantle at depth. populate the South American continent. In Because no earthquake source is needed, the addition, there have been a large number of technique can produce accurate cross sec- portable broadband deployments producing tions from local to unprecedented continen- seismic data across South America. tal scales. The recent increase in instrumentation Workshop participants included a wide paired with growing interest from individual range of scientists at different career stages, network operators to expand the scope of their including seismic network operators, gradu- Kevin Ward seismic research capabilities has opened up ate students, postdoctoral researchers, and the possibility of new collaborations with U.S. professors. Time spent during the workshop research institutions. With the ambitious goal was split between presentations focusing on of extending the recent seismic imaging suc- developing an understanding of the ANT Map of the South American continent showing known cesses of EarthScope to the South American methodology and work time for the partici- seismic stations appropriate for an ambient noise tomog- continent, the Multiscale Imaging of Modern pants to apply what they learned to their raphy (ANT) study. Portable station deployments are Orogenic South America (MIMOSA) project, own data sets. In addition, the International shown as red circles, and permanent stations are shown funded by the U.S. National Science Founda- Development Seismology section of the as yellow circles. Although significant spatial and tempo- tion, aims to develop these mutually beneficial Incorporated Research Institutions for Seis- ral gaps still exist with the current station geometry, the international collaborations (see http://bit.ly/ mology (IRIS) included a presentation that potential for extending a continental-scale ANT study 1TWPaYp). helped make all participants aware of the ser- across South America is rapidly becoming a possibility. Earth & Space Science News Eos.org // 7
MEETING REPORT Norway and Cuba Evaluate Bilateral Climate Research Results XCUBE Workshop Camagüey, Cuba, 16–18 November 2015 gian Embassy in Cuba sees the contribution of researchers from Camagüey as an important part of the XCUBE project; the workshop and field visits were key to the collaboration. In addition, the World Food Program repre- sentatives in Cuba have expressed inter- est in the results of the ongoing (and upcoming) research, which are relevant for their food security assessment in Cuba. Juan Carlos Antuña-Sánchez The lessons learned from the XCUBE project and the workshop discus- sions have provided the framework for a The Grupo de Óptica Atmosférica de Camagüey instruments at Camagüey Meteorological Centre in Camagüey, Cuba. From left to right, the C imel- new proposal for the 318 Sun photometer and the suction nose for the low-volume particle impactor are on the red roof of the instrument control room (small white struc- continuation of ture). The GPS automatic meteorological station is the white cylindrical instrument behind and slightly to the right of the control room. The white XCUBE cooperation, sphere in the center rear is the RD-200SX Doppler radar, designed and built by the National Radar Center in Camagüey. The small gray dome on the which will have a far right is a GPS antenna. major focus on the hydrological effects of climate change S ince 2013, the Future of Climate Weather Forecasts Reanalysis (ERA)-Interim and future food security for Cuba. Alan Robock Extremes in the Caribbean (XCUBE) Reanalysis for Cuba was also discussed (see from Rutgers University (New Brunswick, N.J.) project has studied the vulnerability of http://bit.ly/ERA-Interim). will be leading the work on food security with the Caribbean to future climate extremes. The results achieved are encouraging the cooperation of Roger Rivero Vega from XCUBE is funded by the Norwegian Directorate because they identify, quantify, and make pre- INSMET/Camagüey, an expert on potential cli- for Civil Protection on assignment of the Nor- liminary attribution of ERA-Interim Reanaly- mate change effects on food production. We wegian Ministry of Foreign Affairs. In Novem- sis biases for Cuba. For example, the study expect that this and the next phase of the ber 2015, the Grupo de Óptica Atmosférica de found that 2 -meter surface air temperature in project will enhance scientific understanding Camagüey (GOAC; http://www.goac.cu) of the the ERA-Interim model is warmer than of climate variability in the Caribbean. Cuban Meteorological Institute (INSMET) observed. Further work will be conducted to hosted an XCUBE workshop at which compare temperature at mandatory levels researchers discussed advances in bilateral from Caribbean sounding stations (based on By Juan Carlos Antuña-Marrero, Grupo de scientific cooperation between Cuba and Nor- the Integrated Global Radiosonde Archive data Óptica Atmosférica de Camagüey, Meteo- way on climate change. set) and ERA-Interim Reanalysis. rological Institute, Camagüey, Cuba; email: Workshop participants discussed a recently The workshop also included a visit to the anadelia@caonao.cu; Michel d. S. Mesquita, Uni published paper on sea surface temperature Camagüey Meteorological Centre (CMC), the Research Climate and the Bjerknes Centre for trends in observations and models for the GOAC facilities, the National Radar Center, the Climate Research, Bergen, Norway; and Albeth Caribbean and the Antilles. A follow-up study CMC Forecast Department, and a local facility Rodriguez, Grupo de Óptica Atmosférica de looking at an intercomparison of station data developed jointly by Norway and Cuba to con- Camagüey, Meteorological Institute, Camagüey, and European Centre for M edium-Range duct capacity-building activities. The Norwe- Cuba 8 // Eos 1 July 2016
Creating Career Paths for African-American Students in Geosciences By Robert Liebermann, Lars Ehm, and Gabriel Gwanmesia O n the morning of 6 February 2015, Melissa Sims walked the short path to the podium in the lec- ture hall of the newly constructed National Synchro- tron Light Source II facility, a build- ing of Brookhaven National Labora- tory. This was no ordinary lecture. At age 28, Sims was a graduate student studying how feldspar minerals com- press during meteorite impacts. In the audience sat Secretary of Energy Ernest Moniz, whom she was tasked with introducing at the new facility’s dedication. It’s not every day that a graduate student gets to open for a cabinet member. Rarer still is Sims, an African-American woman geoscien- tist in a field dominated by white men. As she sat on stage, Sims Mmdi/Getty Images Earth & Space Science News Eos.org // 9
ences to A frican-Americans in the 5-year period of 2000–2004. The dearth of degrees awarded to African- Americans is even more pronounced at the master’s level, despite the fact that more than 500,000 such degrees are awarded each year in the United States. As the report notes, “The geosciences have the unenviable distinction of having the poorest representation of Brookhaven National Laboratory African Americans (1%) among master’s degree recipients” [Czujko et al., 2008]. Framework for Training and Employment To address this poor record, the National Sci- ence Foundation (NSF) Directorate for Geosci- ences established in 2006 a program called Opportunities for Enhancing Diversity in the Melissa Sims from Stony Brook University (right) introducing Secretary of Energy Ernest Geosciences (OEDG). Stony Brook’s new ini- Moniz (left) at the dedication of the National Synchrotron Light Source (NSLS) II facility in tiative is a product of OEDG. February 2015 with NSLS director Steve Dierker (far right) looking on. The initiative has a few key steps. First, project leaders seek to recruit undergraduate science and engineering students from under- remembers thinking, “How did I end up here, on a stage represented groups into the graduate program with someone appointed by the president?” in the Department of Geosciences at Stony Brook Univer- Sims is the product of a new initiative at Stony Brook sity. For expediency, efforts are focused on historically University called “A Career Path for African-American black colleges and universities, such as Delaware State Students from Historically Black Colleges and Universities University. to National Laboratories.” The initiative teaches market- Next, the recruited students take courses and develop able skills, places students in internships, and fosters the research projects toward an M.S. in geosciences instru- professional career tracks of underrepresented minorities. mentation—a degree provided by Stony Brook. Thus far, We offer this initiative as a proof of concept example of project leaders have chosen to focus on instrumentation so how and what institutions can do to address the shortage that students could develop marketable skill sets in an of A frican-Americans in the geosciences. emerging field between science and technology. Finally, students receive training that prepares them for The Scope of Underrepresentation employment as science associates in national user facilities The geosciences have the lowest African-American repre- of the U.S. Department of Energy. All graduates of the pro- sentation of all the science, technology, engineering, and gram have conducted their research projects at the mathematics disciplines [Huntoon et al., 2015]. National Synchrotron Light Source (NSLS) of the Brookha- A report from the American Institute of Physics entitled ven National Laboratory (BNL). “Untapped Talent: The African American Presence in Physics and the Geosciences” [Czujko et al., 2008] gives Building on Existing Foundations some background on the root causes of this underrepre- The new program has taken advantage of the long- sentation. standing relationship between professors from historically The report emphasizes that although many African- black colleges and universities and BNL. An important ele- American students have the necessary high school back- ment of this relationship is the Interdisciplinary Consor- grounds to succeed in physics, “these prepared students tium for Research and Educational Access in Science and are more likely to choose math or sciences other than Engineering (INCREASE), an organization that supports physics and geosciences.” In fact, “compared to other sci- access to research facilities not typically available to fac- entific disciplines, physics and the geosciences consis- ulty at historically black colleges and universities (see tently come out near the bottom in terms of their ability to http://www.increaseonline.org/). To enhance its ability to attract and retain African Americans,” the report notes attract A frican-American undergraduates, Stony Brook [Czujko et al., 2008]. For example, in 2004, 4% of African- University has capitalized on its connection with col- American undergraduates earned a bachelor’s degree in leagues in INCREASE institutions to help identify and physics and only 2% in the geosciences (compared with recruit students. 9% for all sciences, which is still below the 13% of African- In addition to I NCREASE and NSLS at BNL, partners in Americans in the U.S. population). this new initiative include the Center for Inclusive Educa- Czujko et al. [2008] also examine the state of African- tion and the Graduate School of Stony Brook University Americans within the larger context of the U.S. educational (see http://bit.ly/1Zc41hJ). All of these organizations have system and social structure, including geography and eco- provided matching funds to complement the National Sci- nomics. Most African-American students go to college ence Foundation support. near their homes, and more than 70% of U.S. universities The M.S. in geosciences instrumentation program and colleges awarded no bachelor’s degrees in the geosci- includes both formal courses and hands-on research proj- 10 // Eos 1 July 2016
Lars Ehm (left to right) Melissa Sims, Adairé Heady, and Ashley Thompson examining one of NSLS’s beamlines. Beamlines are paths for accelerated particles, used in this case to study properties of crystal structures. ects at the NSLS. The projects typically involve the study of returning to his home institution to teach for a year before the physical and chemical properties of minerals under deciding whether to pursue further graduate study. high-pressure conditions, which is the major focus of the Stony Brook’s program shows how science-minded stu- Consortium for Materials Properties for Research in Earth dents, through mentoring and research opportunities, can Sciences, which operates synchrotron beamlines for high- change their expectations to embrace geoscience research. pressure research in the United States. For example, Sims was an undergraduate in exploration geo- physics and headed toward a career in the oil industry. But Program Successes when she learned about Stony Brook’s program, she shifted To date, the initiative has graduated three M.S. students: her ambitions to a more academic direction. Similarly, Ashley Thompson from Delaware State University, Melissa Rhymer initially was considering opportunities in engineer- Sims from the University of South Carolina, and Adairé ing but changed his focus to study geophysics after spending Heady from Delaware State University. All graduated from two summers at BNL in the Science Undergraduate Labora- Stony Brook within a 2-year period. tory Internship program (see http://1.usa.gov/1XOleiB). Thompson is now in a Ph.D. program in mechanical engineering at Stony Brook; Sims, who was awarded a The Future prestigious graduate fellowship from Stony Brook, is The NSF Directorate for Geosciences has approved a studying for her doctorate in geosciences at the university; no-cost extension of Stony Brook’s grant, which allows the and Heady is seeking employment at a national laboratory program’s time period to run to 2016. Unfortunately, NSF such as BNL. has temporarily suspended funding for the OEDG program, In September 2014, Brandon Rhymer from the Univer- so Stony Brook is seeking new funding to extend the pro- sity of the Virgin Islands enrolled in Stony Brook’s initia- gram beyond 2016. However, both Brookhaven National tive. He graduated with his M.S. degree in May 2016 and is Laboratory and the Graduate School at Stony Brook have extended their funding for another 2 years. For tips on how to implement such a program in your institution, contact Robert Liebermann. References Czujko, R., R. Ivie, and J. H. Stith (2008), Untapped talent: The African American pres- ence in physics and the geosciences, Publ. R-444, 22 pp., Am. Inst. of Phys., College Park, Md. Huntoon, J. E., C. Tanenbaum, and J. Hodges (2015), Increasing diversity in the geosci- ences, Eos, 96, doi:10.1029/2015EO025897. Author Information Gabriel Gwanmesia Robert Liebermann, Department of Geosciences and Mineral Physics Institute, Stony Brook University, Stony Brook, N.Y.; email: robert.liebermann@stonybrook.edu; Lars Ehm, Mineral Physics Institute, Stony Brook University, Stony Brook, N.Y., Brandon Rhymer with the 2000-ton uniaxial split sphere apparatus in and Brookhaven National Laboratory, Upton, N.Y.; and Gabriel the Stony Brook High Pressure Laboratory. The apparatus helps scien- Gwanmesia, Department of Physics and Engineering, Dela- tists simulate the high pressures of Earth’s deep interior. ware State University, Dover Earth & Space Science News Eos.org // 11
UNDERSTANDING VOLCANIC ERUPTIONS WHERE PLATES MEET By Raffaele Azzaro and Rosanna De Rosa A new project clarifies the relationships between tectonics and volcanic systems and how they influence hazards on Italy’s Mount Etna and Vulcano and Lipari islands. Mount Etna erupting at dusk. 12 // Eos 1 July 2016
M ount Etna and the Aeo- a cluster of volcanoes, some of the most active lian Islands in southern in Europe. Italy represent ideal nat- The region’s proximity to major urban centers ural laboratories to study is a double-edged sword. Researchers have little how magma and tectonics trouble visiting volcanoes to study how tectonics Antonio Zimbone/AGF/UIG/Getty Images interact in active volcanic influence volcanic plumbing. At the same time, zones and their associated hazards. The geo- this proximity presents hazards to inland com- dynamic context of both areas is characterized munities and those on nearby shores. by a tectonic compression running north and To take advantage of this natural laboratory south, related to the convergence of the Afri- and to help protect people living nearby, sev- can and Eurasian plates in the central Medi- eral branches of Italy’s government research terranean (Figure 1). This compression creates community established the V3 Project—so Earth & Space Science News Eos.org // 13
R. Azzaro The active crater of Vulcano (in the background) viewed from Lipari, in Italy’s Aeolian Islands. The cliffs in the foreground are governed by tectonics. named because it is project number 3 of the Italian Civil frequent, but also the volcano emits a greater volume of Protection Department’s Volcanological Research Pro- lava. gram. Data collection for the project ran from 2012 to At Vulcano and Lipari, in the Aeolian Islands, volcanic 2015; now researchers are analyzing the data to build bet- unrest is much less frequent but produces more intense ter hazards maps and strengthen understanding of how explosive activity and emissions of viscous and thick lava tectonic and volcanic processes work together to exacer- flows. The previous outbreak at Lipari, in 1230, produced a bate risk. renowned eruption of pumice and obsidian. Vulcano erupted more recently, in 1888–1890, but since then it has Tectonic Setting exhibited only high-temperature fumarolic activity. A remnant of the Ionian slab (African plate) is subducting The hazards in active volcanic areas are generally related toward the northwest beneath the Calabrian Arc, which to eruptive activity: lava and flows of hot gas and rock, forms the toe of Italy’s boot [Gvirtzman and Nur, 2001]. The tephra fallout, fast moving mudflows (lahars), or volcanic resulting Tindari Fault is a right-lateral strike-slip struc- gas emissions. However, other less devastating kinds of ture capable of generating moderate earthquakes (the most events may also threaten local communities living on the recent event, in 1978, was M6.2) that extends from the flanks of a volcano, mostly because these events occur fre- central sector of the Aeolian Archipelago (islands of Vul- quently or almost continuously. cano and Lipari) in the southern Tyrrhenian Sea toward the At Etna, recurrent v olcano-tectonic seismicity poses a Etna region to the south [Billi et al., 2006]. This tectonic serious hazard to the 400,000 or so people who live in feature, located in eastern Sicily, is considered to represent urbanized areas and to important infrastructure (roads, a stress transfer zone between the two volcanic areas water/gas/power lines, hospitals, schools, etc.) [Azzaro [De Guidi et al., 2013]. et al., 2016]. At Vulcano, rockfalls and landslides affect- ing the active crater put the village and its tourist facili- A System of Volcanoes ties at risk [Marsella et al., 2015]. These instabilities can Mount Etna (3340 meters above sea level) is the most happen unexpectedly because of variations in volcanic active volcano in Europe. It features nearly constant sum- activity or such other triggering processes as rainfall and mit activity and frequent flank eruptions, with extended seismic activity. Ongoing sea flooding in Lipari’s main lava flows and copious ashfall. Its activity has increased town provides overwhelming evidence of land subsid- significantly in recent years—not only are eruptions more ence that, coupled with the expected sea level rise in the 14 // Eos 1 July 2016
Modified from Billi et al. [2006] Fig. 1. (a) Tectonic map showing the geodynamic framework of the Mediterranean region. (b) Main structural features of Sicily and location of the vol- canic areas studied in the V3 Project. next decades [Anzidei et al., 2014], will lead to future per- The V3 Project had four goals: manent inundations. • nic to define the tectonic framework controlling the volca- systems Addressing the Issues To tackle hazards and risk in this seismically active volca- • mental datatheacquired to analyze exceptionally long time series of instru- by the multiparametric monitoring nic zone, the Italian Civil Protection Department (DPC), and define the relationships among them with the National Institute of Geophysics and Volcanology (INGV, through branches in Catania, Palermo, and Rome), • between to characterize processes connected with the interaction tectonic structures and volcanic systems three Italian universities (Cosenza, Catania, and Rome), and the National Institute of Oceanography and Experi- • of earthquakes, to produce hazards maps aimed at mitigating the effects landslides, and land subsidence mental Geophysics (Trieste), launched the V3 Project. According to the project’s mission statement, V3 aimed The results of the project have been presented at confer- to develop “multidisciplinary analysis of the relationships ences and are being published in technical reports [Azzaro between tectonic structures and volcanic activity.” The and De Rosa, 2016] and scientific papers. project extended previous research programs on the same areas funded by DPC. It dealt with various methodological Assessing Hazards at Etna approaches—tectonic, geophysical, geochemical, petro- As a result of the V3 Project, we now have a greater under- logical, and geotechnical investigations—to interpret standing of the volcanic and tectonic mechanisms that ongoing phenomena and assess related hazards. drive hazards in the region. We found significant correla- tions in the eastern flank of Etna among active fault zones, seismic patterns, variations of crustal geodetic strain, and fluids circu- lation. This opens new perspec- tives to understand faulting at Etna. We have obtained an ana- lytical estimation of creep pro- cesses, indicating that about 40% of the deformation occurs aseis- mically. Moreover, we recognized that the pore pressure of fluids circulating in the volcanic rocks (chiefly groundwater) depends on variations in the crustal strains related to volcanic or seismic M. Anzidei activity [Mattia et al., 2015]. We performed a full probabi- Scientists measure land subsidence effects along the shoreline of Lipari. listic seismic hazards assessment Earth & Space Science News Eos.org // 15
at Etna through local seismic sources defined with instrumental and historic earthquake data sets [Azzaro et al., 2015]. The obtained estimations (Figure 2) show that relevant val- ues of ground accelerations are probabilisti- cally likely to occur also in short times (5–30 years) and are intended to complement the 50-year seismic hazards map of Italy [Stucchi et al., 2011]. The assessment can be used to establish priorities for seismic retrofitting of the more exposed municipalities. V3 efforts improved knowledge of the geometry and structural setting of the sedi- mentary basement underlying Etna using high-resolution aeromagnetic surveys and offshore seismic profiles. They reveal mag- netic anomalies associated with important faults [Nicolosi et al., 2014] and shallow-seated batches of crystallized magma in a framework of active compressive and extensional tectonic structures related to the African plate colliding C. Federico with Europe [Polonia et al., 2016]. Hazards Elsewhere Scientists sample bubbling gases from mofettes—vents where chiefly carbon dioxide The regional pattern of north–south crustal escapes—around Etna. shortening in the southern sector of the Aeo- lian Islands is associated with a diffuse sub- sidence [Esposito et al., 2015], but at a local scale the dynamics reflect different processes (Figure 3a). At Vulcano a shallow (4-kilometer-deep) deflating magmatic source in the northernmost part of the island is periodically fed by deep fluids coming from the underlying reservoir. At Lipari, long- term land subsidence [Anzidei et al., 2016] is enhanced by coastal dynamics (retreating of submarine canyons into the shelf), with a maximum sea level rise of up to 2.2 meters expected in 2100. We confirmed the existence of a common plumbing system responsible for the historic eruptions (less than 1000 years ago) of Lipari and Vulcano. This plumbing system, which lies at a depth of 20 kilometers, periodically feeds shallow magma storage zones where processes of magma crystallization occur [Fusillo et al., 2015]. The eruptive activity took place contemporaneously at both islands along a narrow zone characterized by a domi- nant east–west extensional stress field (Fig- ure 3b). Any future eruption is likely to take place in this narrow zone [Ruch et al., 2016]. The susceptibility of the active crater of Vulcano to landslides, which endanger the main village, is enhanced by hydrothermal alteration of rock mass due to hydrothermal fluid circulation (fumarolic fields, indicated by red in Figure 3a). Fractures and volcano strati- graphic discontinuities control the locations of areas potentially affected by shallow (debris avalanches/flows and rockfalls) and deep- seated instability processes [Cangemi et al., 16 // Eos 1 July 2016
Full assessments can be found on V3’s Web pages (http://bit.ly/ 20Ss8mk). References Anzidei, M., et al. (2014), Coastal structure, s ea- level changes and vertical motion of the land in the Mediterranean, Geol. Soc. Spec. Publ., 388, 453–479, doi:10.1144/SP388.20. Anzidei, M., et al. (2016), New insights on the sub- sidence of Lipari island (Aeolian Islands, southern Italy) from the submerged Roman age pier at Marina Lunga, Quat. Int., 401, 162–173, doi:10.1016/j.quaint.2015.07.003. Azzaro, R., and R. De Rosa (2016), Project V3: Multi-disciplinary analysis of the relationships between tectonic structures and volcanic activity Azzaro and De Rosa [2016] (Etna, Vulcano-Lipari system), final report, Misc. INGV 29, 1722 pp., Ist. Naz. di Geofiz. e Vulcanol., Rome. [Available at https://sites.g oogle.com/a/ ingv.it/volcpro2014/.] Azzaro, R., et al. (2015), Towards a new generation of seismic hazard maps for the volcanic region of Mt. Etna, in Proceedings of the 34° GNGTS Meeting, 17–19 November 2015, Trieste (Italy), pp. 5–11, Ist. Naz. di Oceanogr. e di Geofis. Sper., Fig. 2. (a) Shallow (depth ≤5 kilometers) seismicity recorded at Mount Etna from 2005 to 2014 (circles) Trieste, Italy. and main historic, damaging earthquakes (stars) occurring since 1600. Areas enclosed in yellow lines Azzaro, R., S. D’Amico, and T. Tuvè (2016), Seismic hazard assessment in the volcanic region of indicate the studied seismic zones embracing active faults (black lines): FF, Fiandaca; MF-SLF, Mt. Etna (Italy): A probabilistic approach based Moscarello–San Leonardello; PF, Pernicana; STF-SVF, Santa T ecla–Santa Venerina. (b) Example of on macroseismic data applied to volcano- tectonic seismicity, Bull. Earthquake Eng., probabilistic seismic hazards map: spectral acceleration at 0.2 second, probability of exceedance of doi:10.1007/s10518-015-9806-2, in press. 10% calculated for an exposure time of 50 years. (c) Relevance of local site amplification effects on the Billi, A., et al. (2006), Tectonics and seismicity of maximum value of expected acceleration due to shaking. Colors in Figures 2b and 2c represent the the Tindari Fault System, southern Italy: Crustal deformations at the transition between ongoing values of estimated ground acceleration, from red (maximum) to blue (minimum, close to zero). contractional and extensional domains located above the edge of a subducting slab, Tecton- ics, 25, TC2006, doi:10.1029/2004TC001763. Cangemi, M., et al. (2016), Shallow hydrothermal alteration and permeability changes in pyro 2016]. This makes large rock volumes prone to slide sud- clastic deposits: A case study at La Fossa cone (Vulcano Island, Italy), Geophys. Res. denly, as occurred in 1988. Abstr., 18, EGU2016-2821-1. De Guidi, G., et al. (2013), Multidisciplinary study of the Tindari Fault (Sicily, Italy) sepa- rating ongoing contractional and extensional compartments along the active A frica– Science to Mitigate Risk Eurasia convergent boundary, Tectonophysics, 588, 1–17, doi:10.1016/j.tecto.2012.11.021. Similar to other coordinated research funded by DPC, the Esposito, A., et al. (2015), Eighteen years of GPS surveys in the Aeolian Islands (southern Italy): Open data archive and velocity field, Ann. Geophys., 58, S0439, doi:10.4401/ findings of the V3 Project represent the efforts of the sci- ag-6823. entific community to provide authorities with appropriate Fusillo, R., et al. (2015), Deciphering post-caldera volcanism: Insight into the Vulcanello instruments to mitigate risks in volcanic areas. To do this, (Island of Vulcano, southern Italy) eruptive activity based on geological and petrological constraints, Bull. Volcanol., 77, 76, doi:10.1007/s00445-015-0963-6. V3 endeavored to improve knowledge on inadequately Gvirtzman, Z., and A. Nur (2001), Residual topography, lithospheric structure and sunken studied processes. slabs in the central Mediterranean, Earth Planet. Sci. Lett., 187, 117–130, doi:10.1016/ S0012-821X(01)00272-2. Marsella, M., et al. (2015), Terrestrial laser scanning survey in support of unstable slopes analysis: The case of Vulcano Island (Italy), Nat. Hazards, 78, 443–459, doi:10.1007/s11069-015-1729-3. Mattia, M., et al. (2015), A comprehensive interpretative model of slow slip events on Mt. Etna’s eastern flank, Geochem. Geophys. Geosyst., 16, 635–658, doi:10.1002/2014GC005585. Nicolosi, I., et al. (2014), Volcanic conduit migration over a base ment landslide at Mount Etna (Italy), Sci. Rep., 4, 5293, doi:10.1038/ srep05293. Polonia, A., et al. (2016), The Ionian and Alfeo-Etna fault zones: New Modified from Ruch et al. [2016] segments of an evolving plate boundary in the central Mediterranean Sea?, Tectonophysics, 675, 69–90, doi:10.1016/j.tecto.2016.03.016. Ruch, J., et al. (2016), Magmatic control along a strike-slip volcanic arc: The central Aeolian arc (Italy), Tectonics, 35, 407–424, doi:10.1002/ 2015TC004060. Stucchi, M., et al. (2011), Seismic hazard assessment (2003–2009) for the Italian building code, Bull. Seismol. Soc. Am., 101(4), 1885–1911, doi:10.1785/0120100130. Fig. 3. The Vulcano-Lipari system (Aeolian Islands). (a) Location of the regional (Tindari Author Information Fault zone, responsible for the M6.2 1978 earthquake) and volcanic sources acting in Raffaele Azzaro, Osservatorio Etneo, Istituto this region. Red squares with connected lines are GPS and electronic distance mea- Nazionale di Geofisica e Vulcanologia, Catania, surement networks; blue triangles are leveling benchmarks. (b) Sketch to explain the Italy; email: raffaele.azzaro@ingv.it; and Rosanna transition from strike-slip kinematics along the Tindari Fault (horizontal tectonic stress De Rosa, Dipartimento di Scienze della Terra, (σ1t) dominant) to extension (vertical magmatic stress (σ1m) dominant, orange in Fig- Università della Calabria, Arcavacata di Rende ure 3a) responsible for magma intrusions in the past 20,000 years. (CS), Italy Earth & Space Science News Eos.org // 17
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